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200 papers

We present results of deep surveys of three extragalactic fields, M81 (exposure of 9.7 Ms), LMC (6.8 Ms) and 3C 273/Coma (9.3 Ms), in the hard X-ray (17-60 keV) energy band with the IBIS telescope onboard the INTEGRAL observatory, based on…

IGR J16351-5806 has been associated with the Seyfert 2 galaxy ESO 137-G34, having been first reported as a high energy emitter in the third INTEGRAL/IBIS survey. Using a new diagnostic tool based on X-ray column density measurements vs…

Astrophysics of Galaxies · Physics 2009-11-13 A. Malizia , L. Bassani , F. Panessa , A. De Rosa , A. J. Bird

We present a systematic X-ray study of eight AGNs with intermediate mass black holes (M_BH 8-95x10^4 Msun) based on 12 XMM-Newton observations. The sample includes the two prototype AGNs in this class - NGC4395 and POX52 and six other AGNs…

Astrophysics · Physics 2009-11-13 G. C. Dewangan , S. Mathur , R. E. Griffiths , A. R. Rao

We present an updated mid-infrared (MIR) versus X-ray correlation for the local active galactic nuclei (AGN) population based on the high angular resolution 12 and 18um continuum fluxes from the AGN subarcsecond MIR atlas and 2-10 keV and…

Astrophysics of Galaxies · Physics 2015-10-07 D. Asmus , P. Gandhi , S. F. Hoenig , A. Smette , W. J. Duschl

We find a very strong correlation between the intrinsic spectral slope in X-rays and the amount of Compton reflection from a cold medium in Seyfert AGNs and in hard state of X-ray binaries with either black holes or weakly-magnetized…

Astrophysics · Physics 2009-10-31 A. A. Zdziarski , P. Lubiski , D. A. Smith

We review observations and theoretical models of X-ray/gamma-ray spectra of radio-quiet Seyfert galaxies and of Galactic black-hole candidates (in the hard spectral state). The observed spectra share all their basic components: an…

We have observed with XMM-Newton four radiatively efficient active type 1 galaxies with black hole masses < 10^6 Msun, selected optically from the SDSS. We show here that their soft X-ray spectrum exhibits a soft excess with the same…

Astrophysics · Physics 2009-11-13 G. Miniutti , G. Ponti , J. E. Greene , L. C. Ho , A. C. Fabian , K. Iwasawa

The X-ray properties of Active Galactic Nuclei (AGNs) depend on their underlying physical parameters, particularly the accretion rate. We identified eight reverberation-mapped AGNs with some of the largest known accretion rates without…

High Energy Astrophysical Phenomena · Physics 2024-01-17 Jaya Maithil , Michael S. Brotherton , Ohad Shemmer , Bin Luo , Pu Du , Jian-Min Wang , Hu Chen , Sarah C. Gallagher , Yan-Rong Li , Rodrigo S. Nemmen

X-ray luminosities and spectral indices of 97 bright Seyfert 1 galaxies from XMM archive are analyzed in this article. Distribution of these values is random so we conclude that the model of emission should be at least two-parametric.…

Astrophysics of Galaxies · Physics 2018-12-12 V. A. Sadova , A. V. Tugay

We present photoionization models accounting for both photoelectric and resonant absorption. We demonstrate that resonance absorption lines are detectable even in moderate resolution X-ray spectra of type 1 AGN. The spectra transmitted by…

Astrophysics · Physics 2007-05-23 F. Nicastro , F. Fiore , G. Matt

I present ASCA observations of IRAS00317-2142, the most luminous (Lx~10^43 erg s-1 0.1-2 keV) of the 'composite' class of galaxies. This enigmatic class of objects presents narrow-emission line optical spectra classifying these galaxies as…

Astrophysics · Physics 2009-10-31 I. Georgantopoulos

We present mid-infrared data of a sample of 57 AGNs obtained with the instrument ISOCAM on board the satellite ISO. The images were obtained through the LW2 (6.75 microns) and LW7 (9.62 microns) filters. This is a new analysis of Clavel et…

We present the results of the X-ray spectral analysis of the first deep X-ray survey with the XMM-Newton observatory during Performance Verification. We restrict the analysis to the sample of 98 sources with more than 70 net counts (flux…

Astrophysics · Physics 2009-11-07 V. Mainieri , J. Bergeron , G. Hasinger , I. Lehmann , P. Rosati , M. Schmidt , G. Szokoly , R. Della Ceca

We present a systematic X-ray study, the third in a series, of 49 active galactic nuclei with intermediate-mass black holes (IMBH; ~10^5-10^6 M_sun) using Chandra observations. We detect 42 out of 49 targets with a 0.5-2 keV X-ray…

Astrophysics of Galaxies · Physics 2015-06-11 Ruobing Dong , Jenny E. Greene , Luis C. Ho

Narrow Line Seyfert 1 galaxies (NLS1) are very interesting objects which display peculiar properties when compared to their broad line analogues (BLS1). Although well studied in many wavebands, their behaviour at >10 keV is poorly studied…

In this letter we present the primary continuum parameters, the photon index Gamma and the high energy cut-off Ec, of 41 type-1 Seyfert galaxies extracted from the INTEGRAL complete sample of AGN. We performed a broad band (0.3-100 keV)…

High Energy Astrophysical Phenomena · Physics 2015-06-18 A. Malizia , M. Molina , L. Bassani , J. B. Stephen , A. Bazzano , P. Ubertini , A. J. Bird

The masses of 68 supermassive black holes (SMBHs) in nearby (z<0.15) active galactic nuclei (AGNs) detected by the INTEGRAL observatory in the hard X-ray energy band (17-60 keV) outside the Galactic plane (|b| > 5 degrees) have been…

Cosmology and Nongalactic Astrophysics · Physics 2012-10-24 G. A. Khorunzhev , S. Yu. Sazonov , R. A. Burenin , A. Yu. Tkachenko

Multiwavelength observations are essential to constrain physical parameters of the blazars observed by Fermi/LAT. Among the 187 AGN significantly detected in public INTEGRAL data above 20 keV by the imager IBIS/ISGRI, 20 blazars were…

High Energy Astrophysical Phenomena · Physics 2009-12-14 V. Beckmann , C. Ricci , S. Soldi

We report on the iron K-alpha line properties of a sample of Seyfert galaxies observed with the XMM-Newton EPIC pn instrument. Using a systematic and uniform analysis, we find that complexity at iron-K is extremely common in the XMM…

Astrophysics · Physics 2010-11-11 K. Nandra , P. M. O'Neill , I. M. George , J. N. Reeves , T. J. Turner

We present results from Chandra observations of 14 ultraluminous infrared galaxies (ULIRGs; log(L_IR/L_Sun) >= 12) with redshifts between 0.04 and 0.16. The goals of the observations were to investigate any correlation between infrared…

Astrophysics · Physics 2009-11-13 Stacy H. Teng , A. S. Wilson , S. Veilleux , A. J. Young , D. B. Sanders , N. M. Nagar